We see that the black hole has two horizons. As \(q\longrightarrow 0\) 
the horizon of the squashed Kaluza- Klein Gödel black hole is
recovered [1]} and when \(q\)  and \(j\)  tend to zero, we have
\(r_{h}^2=2M\) , which is the horizon of five-dimensional Schwarzschild
black hole. Here we note that the argument of square root
constraints the mass, charge and Gödel parameter values. When
\(r_{\infty }\longrightarrow \infty \) , we have \(k(r)\longrightarrow 1\) ,
which means that the squashing effect
disappears and the five-dimensional charged black hole is recovered.
